141 research outputs found
ΠΠ²ΡΠΎΠΏΠ°, Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠ΅ ΠΈ Π²Π»ΠΈΡΠ½ΠΈΠ΅ ΠΌΠΈΡΠΎΠ²ΠΎΠΉ ΠΏΠΎΠ»ΠΈΡΠΈΠΊΠΈ
Π ΡΠΊΠΎΠΏΠΈΡΡ ΠΏΠΎΡΡΡΠΏΠΈΠ»Π° Π² ΡΠ΅Π΄Π°ΠΊΡΠΈΡ: 28.03.2021. ΠΡΠΈΠ½ΡΡΠ° ΠΊ ΠΏΡΠ±Π»ΠΈΠΊΠ°ΡΠΈΠΈ: 11.05.2021.Received: 28.03.2021. Accepted: 11.05.2021.Π‘ ΡΠ΅Ρ
ΠΏΠΎΡ, ΠΊΠ°ΠΊ ΠΠ²ΡΠΎΠΏΠ΅ΠΉΡΠΊΠΈΠΉ ΡΠΎΡΠ· ΡΡΠ°Π» ΠΈΠ³ΡΠ°ΡΡ ΡΠ°ΡΡΡΡΡΡ ΡΠΎΠ»Ρ Π² ΠΎΡΠ½ΠΎΡΠ΅Π½ΠΈΡΡ
ΠΌΠ΅ΠΆΠ΄Ρ Π³ΠΎΡΡΠ΄Π°ΡΡΡΠ²Π°ΠΌΠΈ-ΡΠ»Π΅Π½Π°ΠΌΠΈ ΠΈ ΡΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠΊΠΈΠΌΠΈ ΡΡΡΠ°Π½Π°ΠΌΠΈ, Π½Π΅ Π²Ρ
ΠΎΠ΄ΡΡΠΈΠΌΠΈ Π² ΠΠ‘, ΠΏΠΎΠ»ΠΈΡΠΈΠΊΠΈ Π² ΠΡΡΡΡΠ΅Π»Π΅ ΡΡΠ°Π»ΠΈ ΡΠ΄Π΅Π»ΡΡΡ Π±ΠΎΠ»ΡΡΠΎΠ΅ Π²Π½ΠΈΠΌΠ°Π½ΠΈΠ΅ ΡΠ°Π·ΡΠ°Π±ΠΎΡΠΊΠ΅ ΠΈ ΡΠ΅Π°Π»ΠΈΠ·Π°ΡΠΈΠΈ Π΄Π΅ΠΉΡΡΠ²ΠΈΠΉ ΠΈ ΠΏΡΠΎΠ³ΡΠ°ΠΌΠΌ, Π½Π°ΠΏΡΠ°Π²Π»Π΅Π½Π½ΡΡ
Π½Π° ΠΏΠΎΠΎΡΡΠ΅Π½ΠΈΠ΅ ΠΌΠΈΡΠ°, ΡΡΠ°Π±ΠΈΠ»ΡΠ½ΠΎΡΡΠΈ ΠΈ ΡΠ°Π·Π²ΠΈΡΠΈΡ Π² ΡΠ΅Π³ΠΈΠΎΠ½Π΅. ΠΡΡΠ΅ΠΊΡ ΠΎΡ ΡΠ°ΠΊΠΎΠ³ΠΎ ΡΡΠ°ΡΡΠΈΡ ΠΎΠΊΠ°Π·Π°Π»ΡΡ Π½Π΅ ΡΡΠΎΠ»Ρ Π·Π½Π°ΡΠΈΡΠ΅Π»ΡΠ½ΡΠΌ, ΠΊΠ°ΠΊ ΠΎΠΆΠΈΠ΄Π°Π»ΠΎΡΡ, Π½ΠΎ, ΡΠ΅ΠΌ Π½Π΅ ΠΌΠ΅Π½Π΅Π΅, ΠΎΡΡΡΠΈΠΌΡΠΌ. ΠΠ°ΠΏΡΡΠΆΠ΅Π½ΠΈΠ΅ ΠΏΠΎΡΡΠΈ Π²ΡΠ΅Π³Π΄Π° Π²ΠΈΡΠ°Π»ΠΎ Π½Π°Π΄ Π²ΠΎΠ΄Π°ΠΌΠΈ Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠ³ΠΎ ΠΌΠΎΡΡ, ΠΏΠΎΡΠΎΠΌΡ ΡΡΠΎ ΠΊΡΠΈΠ·ΠΈΡΡ ΠΈ ΠΆΠ΅ΡΡΠΎΠΊΠΈΠ΅ ΠΊΠΎΠ½ΡΠ»ΠΈΠΊΡΡ ΡΠ»Π΅Π΄ΠΎΠ²Π°Π»ΠΈ ΠΎΠ΄ΠΈΠ½ Π·Π° Π΄ΡΡΠ³ΠΈΠΌ, Π½ΠΎ Π½ΠΈΠΊΠΎΠ³Π΄Π° Π½Π΅ ΡΠ°Π·ΡΡΡΠ°Π»ΠΈ Π²ΡΠ΅ ΠΎΡΠ½ΠΎΡΠ΅Π½ΠΈΡ. ΠΠ°ΡΡΠΎΡΡΠ°Ρ ΡΡΠ°ΡΡΡ ΠΎΡΠ½ΠΎΠ²Π°Π½Π° Π½Π° ΡΡΠΎΠΉ ΠΎΡΠΎΠ±Π΅Π½Π½ΠΎΡΡΠΈ Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΡ ΠΈ ΠΏΡΠ΅Π΄Π»Π°Π³Π°Π΅Ρ Π²Π·Π³Π»ΡΠ½ΡΡΡ Π½Π° ΡΡΠΎΡ ΡΠ΅Π³ΠΈΠΎΠ½ ΠΏΠΎΠ΄ Π΄ΡΡΠ³ΠΈΠΌ ΡΠ³Π»ΠΎΠΌ Π·ΡΠ΅Π½ΠΈΡ. ΠΠΎΠΏΡΠ΅ΠΊΠΈ ΠΏΡΠ΅ΠΎΠ±Π»Π°Π΄Π°ΡΡΠ΅ΠΌΡ ΠΌΠ½Π΅Π½ΠΈΡ ΠΎ Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠ΅ ΠΊΠ°ΠΊ ΠΎ Π·ΠΎΠ½Π΅, Π½Π΅ Π·Π°ΡΡΠΎΠ½ΡΡΠΎΠΉ ΠΈΠ»ΠΈ ΠΏΠΎΡΡΠΈ Π½Π΅ Π·Π°ΡΡΠΎΠ½ΡΡΠΎΠΉ ΠΎΡΠ½ΠΎΠ²Π½ΡΠΌΠΈ ΠΌΠΈΡΠΎΠ²ΡΠΌΠΈ ΡΠΎΠ±ΡΡΠΈΡΠΌΠΈ, Π² ΡΠ°Π±ΠΎΡΠ΅ Π°Π½Π°Π»ΠΈΠ·ΠΈΡΡΠ΅ΡΡΡ Π²Π»ΠΈΡΠ½ΠΈΠ΅ ΠΌΠ΅ΠΆΠ΄ΡΠ½Π°ΡΠΎΠ΄Π½ΡΡ
ΠΈΠ½ΡΡΠΈΡΡΡΠΎΠ² ΠΈ Π΄Π΅ΠΉΡΡΠ²ΠΈΠΉ, Π²Π»ΠΈΡΡΡΠΈΡ
Π½Π° Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠΊΠΈΠΉ ΡΠ΅Π³ΠΈΠΎΠ½. ΠΠ²ΡΠΎΡ ΡΠ°ΠΊΠΆΠ΅ ΠΏΡΠΈΠ²Π»Π΅ΠΊΠ°Π΅Ρ Π²Π½ΠΈΠΌΠ°Π½ΠΈΠ΅ ΡΠΈΡΠ°ΡΠ΅Π»Π΅ΠΉ ΠΊ Π°ΠΊΡΠΈΠ²Π½ΠΎΠΉ, Π° Π² Π½Π΅ΠΊΠΎΡΠΎΡΡΡ
ΡΠ»ΡΡΠ°ΡΡ
β ΠΊ ΠΏΠ°ΡΡΠΈΠ²Π½ΠΎΠΉ ΠΏΠΎΠ·ΠΈΡΠΈΠΈ ΠΏΡΠ°Π²ΠΈΡΠ΅Π»ΡΡΡΠ² ΡΠ΅Π³ΠΈΠΎΠ½Π° Π² ΠΌΠΈΡΠΎΠ²ΡΡ
ΠΈΠ½ΡΡΠΈΡΡΡΠ°Ρ
ΠΈ ΠΌΠ΅ΠΆΠ΄ΡΠ½Π°ΡΠΎΠ΄Π½ΠΎΠΉ ΠΏΠΎΠ»ΠΈΡΠΈΠΊΠ΅. Π‘ΠΎΠΎΡΠ²Π΅ΡΡΡΠ²Π΅Π½Π½ΠΎ, ΠΏΠ΅ΡΠ²ΡΠΉ ΡΠ°Π·Π΄Π΅Π» ΠΏΡΠ΅Π΄Π»Π°Π³Π°Π΅Ρ Π²Π½ΠΈΠΌΠ°Π½ΠΈΡ ΡΠΈΡΠ°ΡΠ΅Π»Π΅ΠΉ ΠΊΠΎΠ½ΡΠ΅ΠΏΡΠΈΠΈ, ΠΏΡΠΈΠ³ΠΎΠ΄Π½ΡΠ΅ Π΄Π»Ρ Π°Π½Π°Π»ΠΈΠ·Π° ΠΌΠΈΡΠ° ΠΊΠ°ΠΊ ΠΏΠΎΠ»ΠΈΡΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ ΠΏΡΠΎΡΡΡΠ°Π½ΡΡΠ²Π°, Π² ΠΊΠΎΡΠΎΡΠΎΠΌ Π±ΡΠ»ΠΈ ΡΠΎΠ·Π΄Π°Π½Ρ ΠΈΠ½ΡΡΠΈΡΡΡΡ Π΄Π»Ρ ΠΏΡΠΎΠ²Π΅Π΄Π΅Π½ΠΈΡ ΠΏΠΎΠ»ΠΈΡΠΈΠΊΠΈ, ΡΠ΅Π°Π³ΠΈΡΡΡΡΠ΅ΠΉ Π½Π° ΠΏΡΠΎΠ±Π»Π΅ΠΌΡ ΠΌΠΈΡΠΎΠ²ΠΎΠ³ΠΎ ΠΌΠ°ΡΡΡΠ°Π±Π°. ΠΠΎ Π²ΡΠΎΡΠΎΠΌ ΡΠ°Π·Π΄Π΅Π»Π΅ ΠΈΠ·Π»Π°Π³Π°ΡΡΡΡ ΠΎΡΠ½ΠΎΠ²Π½ΡΠ΅ ΠΌΠ΅ΠΆΠ΄ΡΠ½Π°ΡΠΎΠ΄Π½ΡΠ΅ ΠΏΠΎΠ΄Ρ
ΠΎΠ΄Ρ ΠΊ Π±Π΅Π·ΠΎΠΏΠ°ΡΠ½ΠΎΡΡΠΈ ΠΈ ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΠ΅ΡΠΊΠΎΠΉ ΠΏΠΎΠ»ΠΈΡΠΈΠΊΠ΅, ΠΊΠΎΡΠΎΡΡΠ΅ Π±ΡΠ»ΠΈ ΡΠ°Π·ΡΠ°Π±ΠΎΡΠ°Π½Ρ Π΄Π»Ρ ΡΠ΅Π°Π³ΠΈΡΠΎΠ²Π°Π½ΠΈΡ Π½Π° ΠΌΠΈΡΠΎΠ²ΡΠ΅ ΠΏΡΠΎΠ±Π»Π΅ΠΌΡ ΠΈ, ΡΠ»Π΅Π΄ΠΎΠ²Π°ΡΠ΅Π»ΡΠ½ΠΎ, Π΄Π»Ρ Π½Π°Π²Π΅Π΄Π΅Π½ΠΈΡ ΠΏΠΎΡΡΠ΄ΠΊΠ° Π² ΠΌΠΈΡΠ΅, Π²ΠΊΠ»ΡΡΠ°Ρ Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠΊΠΈΠΉ ΡΠ΅Π³ΠΈΠΎΠ½. Π ΡΡΠ΅ΡΡΠ΅ΠΌ ΡΠ°Π·Π΄Π΅Π»Π΅ ΠΎΡΠ½ΠΎΠ²Π½ΠΎΠ΅ Π²Π½ΠΈΠΌΠ°Π½ΠΈΠ΅ ΡΠ΄Π΅Π»ΡΠ΅ΡΡΡ ΠΏΡΠΎΠ³Π½ΠΎΠ·ΠΈΡΠΎΠ²Π°Π½ΠΈΡ ΠΌΠΈΡΠΎΠ²ΠΎΠΉ ΠΈ ΡΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠΊΠΎΠΉ ΠΏΠΎΠ»ΠΈΡΠΈΠΊΠΈ Π±Π»ΠΈΠΆΠ°ΠΉΡΠΈΡ
Π»Π΅Ρ Ρ ΡΡΠ΅ΡΠΎΠΌ ΠΏΡΠΎΡΠΈΠ²ΠΎΡΡΠΎΡΠ½ΠΈΡ ΡΡΠ΅Ρ
Π²Π΅Π»ΠΈΠΊΠΈΡ
Π΄Π΅ΡΠΆΠ°Π² β Π‘Π¨Π, ΠΠΈΡΠ°Ρ ΠΈ Π ΠΎΡΡΠΈΠΈ. ΠΡΠ΅ΠΏΡΡΡΡΠ²ΠΈΡ Π΄Π»Ρ ΡΠΎΡ
ΡΠ°Π½Π΅Π½ΠΈΡ Π² Π½Π΅ΠΈΠ·ΠΌΠ΅Π½Π½ΠΎΠΌ Π²ΠΈΠ΄Π΅ Π·Π°ΠΏΠ°Π΄Π½ΠΎΠΉ ΠΊΠΎΠ°Π»ΠΈΡΠΈΠΈ Π½Π΅ ΠΌΠΎΠ³ΡΡ ΠΏΠΎΠΌΠ΅ΡΠ°ΡΡ Π²ΠΎΠ·ΠΎΠ±Π½ΠΎΠ²Π»Π΅Π½ΠΈΡ Π³Π΅Π³Π΅ΠΌΠΎΠ½ΠΈΠΈ Π‘Π¨Π, Π΅ΡΠ»ΠΈ Π±Π΅ΡΠΏΠΎΡΡΠ΄ΠΎΠΊ ΠΎΠΊΠ°ΠΆΠ΅ΡΡΡ Π½Π΅ΠΏΡΠΈΠ΅ΠΌΠ»Π΅ΠΌΡΠΌ Π΄Π»Ρ Π±ΠΎΠ»ΡΡΠΎΠ³ΠΎ ΡΠΈΡΠ»Π° ΡΡΡΠ°Π½. ΠΠΈΡΠ°ΠΉΡΠΊΠ°Ρ ΠΌΠΎΠ΄Π΅Π»Ρ ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΠ΅ΡΠΊΠΎΠΉ ΠΎΡΠΊΡΡΡΠΎΡΡΠΈ ΠΈ Π½Π΅ΠΉΡΡΠ°Π»ΡΠ½ΠΎΡΡΠΈ ΠΊΠΎΠΌΠΏΠ°Π½ΠΈΠΉ-ΠΈΠ½Π²Π΅ΡΡΠΎΡΠΎΠ² ΠΌΠΎΠΆΠ΅Ρ ΡΠ°Π±ΠΎΡΠ°ΡΡ Π½Π΅ Π²ΠΎ Π²ΡΠ΅Ρ
ΡΡΡΠ°Π½Π°Ρ
Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΡ. ΠΠ°ΡΡΡΠ°Ρ ΡΠΏΠΎΠΊΠΎΠΉΡΡΠ²ΠΈΠ΅ ΠΈ ΠΈΠ·ΠΌΠ΅Π½ΡΡ ΠΏΡΠ°Π²ΠΈΠ»Π° ΠΈΠ³ΡΡ Π² ΡΠ»ΠΎΠΆΠ½ΡΡ
ΡΡΠ»ΠΎΠ²ΠΈΡΡ
Π±Π΅Π·ΠΎΠΏΠ°ΡΠ½ΠΎΡΡΠΈ, ΡΠ°ΠΊΠΈΡ
ΠΊΠ°ΠΊ Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠ΅, ΠΏΠΎΠ΄Π΄Π΅ΡΠΆΠΈΠ²Π°Ρ Π°Π²ΡΠΎΡΠΈΡΠ°ΡΠ½ΡΠ΅ ΡΠ΅ΠΆΠΈΠΌΡ, Π ΠΎΡΡΠΈΡ ΡΡΡΠ΅ΠΌΠΈΡΡΡ ΡΠΎΠ·Π΄Π°ΡΡ ΡΠΈΡΡΠ°ΡΠΈΡ, Π² ΠΊΠΎΡΠΎΡΠΎΠΉ Π‘ΠΎΠ΅Π΄ΠΈΠ½Π΅Π½Π½ΡΠ΅ Π¨ΡΠ°ΡΡ ΠΠΌΠ΅ΡΠΈΠΊΠΈ ΠΈ Π΅Π²ΡΠΎΠΏΠ΅ΠΉΡΠΊΠΈΠ΅ ΡΡΡΠ°Π½Ρ Π½Π΅ ΠΌΠΎΠ³Π»ΠΈ Π±Ρ ΠΏΡΠΈΠ½ΠΈΠΌΠ°ΡΡ Π½ΠΈΠΊΠ°ΠΊΠΈΡ
ΡΠ΅ΡΠ΅Π½ΠΈΠΉ Π±Π΅Π· Π΅Π΅ ΡΡΠ°ΡΡΠΈΡ. Π‘ΠΎΠΎΡΠ²Π΅ΡΡΡΠ²Π΅Π½Π½ΠΎ, Π²ΡΠ²ΠΎΠ΄Ρ ΡΡΠ°ΡΡΠΈ ΠΏΡΠΈΠ·ΡΠ²Π°ΡΡ ΠΊ Π½Π°ΠΊΠΎΠΏΠ»Π΅Π½ΠΈΡ Π·Π½Π°Π½ΠΈΠΉ ΠΎ ΡΠ΅ΠΊΠΎΠ½ΡΠΈΠ³ΡΡΠ°ΡΠΈΠΈ ΠΌΠΈΡΠΎΠ²ΡΡ
ΠΊΠΎΠ°Π»ΠΈΡΠΈΠΉ ΠΈ ΠΈΠ·ΠΌΠ΅Π½Π΅Π½ΠΈΠΈ ΠΌΠ΅ΠΆΠ΄ΡΠ½Π°ΡΠΎΠ΄Π½ΠΎΠ³ΠΎ ΠΏΠΎΠ»ΠΎΠΆΠ΅Π½ΠΈΡ. ΠΡΠΎΠ±Π΅Π½Π½ΠΎ ΡΡΠ°ΡΠ΅Π»ΡΠ½ΠΎ ΡΠ»Π΅Π΄ΡΠ΅Ρ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°ΡΡ ΠΏΠΎΠ»ΠΈΡΠΈΠΊΡ ΡΠ΅Π²ΠΈΠ·ΠΈΠΎΠ½ΠΈΠ·ΠΌΠ° ΡΡΠ΅Ρ
Π³ΠΎΡΡΠ΄Π°ΡΡΡΠ², ΡΠΎΡΠ΅Π²Π½ΡΡΡΠΈΡ
ΡΡ Π·Π° ΠΌΠΈΡΠΎΠ²ΠΎΠ΅ Π»ΠΈΠ΄Π΅ΡΡΡΠ²ΠΎ. ΠΠ΅ΡΠ²ΠΎΡΡΠ΅ΠΏΠ΅Π½Π½ΠΎΠ΅ Π·Π½Π°ΡΠ΅Π½ΠΈΠ΅ ΠΈΠΌΠ΅ΡΡ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ Π²Π»ΠΈΡΠ½ΠΈΡ ΡΠ°ΠΊΠΎΠ³ΠΎ Π³Π»ΠΎΠ±Π°Π»ΡΠ½ΠΎΠ³ΠΎ ΠΏΡΠΎΡΠ΅ΡΡΠ° Π½Π° Π±ΠΎΠ»Π΅Π΅ ΠΎΠ±ΡΠΈΡΠ½ΡΠΉ ΡΠ°ΠΉΠΎΠ½ Π‘ΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΡ ΠΈ Π½Π° ΡΡΠ°ΡΡΠΈΠ΅ ΡΡΠ΅Π΄ΠΈΠ·Π΅ΠΌΠ½ΠΎΠΌΠΎΡΡΠΊΠΈΡ
ΡΡΡΠ°Π½ Π² ΡΡΠΎΠΌ ΠΏΡΠΎΡΠ΅ΡΡΠ΅.Since the European Union began to play a growing role in the relationships between the Member States and the Non-EU Mediterranean countries, the policymakers in Brussels have devoted a great deal of attention to devise and implement actions and programmes aimed at promoting peace, stability and growth to the area. The effects of such involvement have been not as signifi cant as expected but not even insignifi cant. Tension has almost always floated over the Mediterranean waters because crises and violent conflicts have followed one another though never breaking all relations down. The present paper takes a cue from this feature of the Mediterranean area and proposes to watch the territory from a different angle of view. Contrary to the prevailing view of the Mediterranean as an area unaffected or scarcely affected by the dominant world policies, the paper analyses the impact of the world policy-making institutions and policies on the Mediterranean area. It also draws the readersβ attention towards the participation and, in significant cases, the non-participation of the governments of the area in the world institutions and policies. Accordingly, the first section highlights the concepts useful to analyze the world as the political space in which policymaking institutions have been established for building policies that respond to world-scale problems. The second section outlines the signifi cant security and economic world policies that have been established for responding to world problems and, consequently, for bringing order to the world, the Mediterranean area included. In the third section, the focus is on forecasting the world and Mediterranean politics of the coming years by drawing the readersβ attention to the confrontation of three big powers, the USA, China and Russia. The difficulty to keep unaltered the Western coalition could not impede the renewal of the US hegemony should disorder be unsustainable to loads of countries. The Chinese model of economic openness and the non-interference of the investing companies may not work in all the Mediterranean countries. By acting as a troublemaker and game-changer in security complex settings like the Mediterranean area by bolstering authoritarian regimes, Russia mostly wants to create a situation in which the United States and the European countries find it impossible to make any decisions without its participation. Accordingly, the paperβs conclusions call for building knowledge about the reconfi guration of the world coalitions and the change of the existing order and institutions. Especially the revisionism of the three states competing for world leadership requires careful investigation. Research on the influence of such a global process on the wider Mediterranean area and the involvement of the Mediterranean countries in such a process is of paramount importance
Evoluzione della sostanza organica in suoli rappresentativi dell'altopiano della Sila
Abstract: Organic-matter evolution of soils from Sila uplands (Calabria, Italy). Soil organic matter (SOM) has long been known for its central role in chemical, biochemical and physiological soil processes. Efforts in optimizing crop production, minimizing environmental pollution, and enhancing soil quality all require a better understanding of the nature and evolution of soil organic matter for its proper management. Four sites (S1 ' S4), developed on an area of about 9000 ha, in the Sila Mountains, were evaluated to study the turnover of the soil organic matter. The SOM of four sites studied undergoes to a fast mineralization process in the sites S1, S3 and S4, a pastureland, a grass-pastureland, and a cropland, respectively. An opposite trend is observed in the S2 site, under mixed forest of coniferous and broadleaf, where prevailed the humification process
PREOPERATIVE EMBOLIZATION OF THYROID ARTERIES IN A PATIENT WITH LARGE NON βHODGKIN THYROID LYNPHOMA
LOFT - a Large Observatory For x-ray Timing
The high time resolution observations of the X-ray sky hold the key to a
number of diagnostics of fundamental physics, some of which are unaccessible to
other types of investigations, such as those based on imaging and spectroscopy.
Revealing strong gravitational field effects, measuring the mass and spin of
black holes and the equation of state of ultradense matter are among the goals
of such observations. At present prospects for future, non-focused X-ray timing
experiments following the exciting age of RXTE/PCA are uncertain. Technological
limitations are unavoidably faced in the conception and development of
experiments with effective area of several square meters, as needed in order to
meet the scientific requirements. We are developing large-area monolithic
Silicon Drift Detectors offering high time and energy resolution at room
temperature, which require modest resources and operation complexity (e.g.,
read-out) per unit area. Based on the properties of the detector and read-out
electronics that we measured in the lab, we developed a realistic concept for a
very large effective area mission devoted to X-ray timing in the 2-30 keV
energy range. We show that effective areas in the range of 10-15 square meters
are within reach, by using a conventional spacecraft platform and launcher of
the small-medium class.Comment: 13 pages, 8 figures, 1 table, Proceedings of SPIE Vol. 7732, Paper
No. 7732-66, 201
Evaluation of clinical, laboratory and morphologic prognostic factors in colon cancer
<p>Abstract</p> <p>Background</p> <p>The long-term prognosis of patients with colon cancer is dependent on many factors. To investigate the influence of a series of clinical, laboratory and morphological variables on prognosis of colon carcinoma we conducted a retrospective analysis of our data.</p> <p>Methods</p> <p>Ninety-two patients with colon cancer, who underwent surgical resection between January 1999 and December 2001, were analyzed. On survival analysis, demographics, clinical, laboratory and pathomorphological parameters were tested for their potential prognostic value. Furthermore, univariate and multivariate analysis of the above mentioned data were performed considering the depth of tumour invasion into the bowel wall as independent variable.</p> <p>Results</p> <p>On survival analysis we found that depth of tumour invasion (P < 0.001; F-ratio 2.11), type of operation (P < 0.001; F-ratio 3.51) and CT scanning (P < 0.001; F-ratio 5.21) were predictors of survival. Considering the degree of mural invasion as independent variable, on univariate analysis, we observed that mucorrhea, anismus, hematocrit, WBC count, fibrinogen value and CT scanning were significantly related to the degree of mural invasion of the cancer. On the multivariate analysis, fibrinogen value was the most statistically significant variable (P < 0.001) with the highest F-ratio (F-ratio 5.86). Finally, in the present study, the tumour site was significantly related neither to the survival nor to the mural invasion of the tumour.</p> <p>Conclusion</p> <p>The various clinical, laboratory and patho-morphological parameters showed different prognostic value for colon carcinoma. In the future, preoperative prognostic markers will probably gain relevance in order to make a proper choice between surgery, chemotherapy and radiotherapy. Nevertheless, current data do not provide sufficient evidence for preoperative stratification of high and low risk patients. Further assessments in prospective large studies are warranted.</p
The Cherenkov Telescope Array: layout, design and performance
The Cherenkov Telescope Array (CTA) will be the next generation very-high-energy gamma-ray observatory. CTA is expected to provide substantial improvement in accuracy and sensitivity with respect to existing instruments thanks to a tenfold increase in the number of telescopes and their state-of-the-art design. Detailed Monte Carlo simulations are used to further optimise the number of telescopes and the array layout, and to estimate the observatory performance using updated models of the selected telescope designs. These studies are presented in this contribution for the two CTA stations located on the island of La Palma (Spain) and near Paranal (Chile) and for different operation and observation conditions
Performance of the Cherenkov Telescope Array in the presence of clouds
The Cherenkov Telescope Array (CTA) is the future ground-based observatory for gamma-ray astronomy at very high energies. The atmosphere is an integral part of every Cherenkov telescope. Different atmospheric conditions, such as clouds, can reduce the fraction of Cherenkov photons produced in air showers that reach ground-based telescopes, which may affect the performance. Decreased sensitivity of the telescopes may lead to misconstructed energies and spectra. This study presents the impact of various atmospheric conditions on CTA performance. The atmospheric transmission in a cloudy atmosphere in the wavelength range from 203 nm to 1000 nm was simulated for different cloud bases and different optical depths using the MODerate resolution atmospheric TRANsmission (MODTRAN) code. MODTRAN output files were used as inputs for generic Monte Carlo simulations. The analysis was performed using the MAGIC Analysis and Reconstruction Software (MARS) adapted for CTA. As expected, the effects of clouds are most evident at low energies, near the energy threshold. Even in the presence of dense clouds, high-energy gamma rays may still trigger the telescopes if the first interaction occurs lower in the atmosphere, below the cloud base. A method to analyze very high-energy data obtained in the presence of clouds is presented. The systematic uncertainties of the method are evaluated. These studies help to gain more precise knowledge about the CTA response to cloudy conditions and give insights on how to proceed with data obtained in such conditions. This may prove crucial for alert-based observations and time-critical studies of transient phenomena
Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events
We investigate the possibility of detection of the VHE gamma-ray counterparts to the neutrino astrophysical sources within the Neutrino Target of Opportunity (NToO) program of CTA using the populations simulated by the FIRESONG software to resemble the diffuse astrophysical neutrino flux measured by IceCube. We derive the detection probability for different zenith angles and geomagnetic field configurations. The difference in detectability of sources between CTA-North and CTA-South for the average geomagnetic field is not substantial. We investigate the effect of a higher night-sky background and the preliminary CTA Alpha layout on the detection probability
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